Final Exam Earth science
... Earth has seasons because its axis is tilted as it moves around the sun causing unequal heating of the Earth’s surface. 2. Day and Night are associated w/the rotation of the Earth around its axis. The side facing the sun is experiencing day. 6. The geographic north pole is the northernmost point on ...
... Earth has seasons because its axis is tilted as it moves around the sun causing unequal heating of the Earth’s surface. 2. Day and Night are associated w/the rotation of the Earth around its axis. The side facing the sun is experiencing day. 6. The geographic north pole is the northernmost point on ...
Fourth Grade Earth in the Universe - K
... • 1.E.1 Recognize the features and patterns of the earth/moon/sun system as observed from Earth. • 1.E.1.1 Recognize differences in the features of the day and night sky and apparent movement of objects across the sky as observed from Earth. • 1.E.1.2 Recognize patterns of observable changes in the ...
... • 1.E.1 Recognize the features and patterns of the earth/moon/sun system as observed from Earth. • 1.E.1.1 Recognize differences in the features of the day and night sky and apparent movement of objects across the sky as observed from Earth. • 1.E.1.2 Recognize patterns of observable changes in the ...
QUIZ 1 - AY5-S13 . . . . . . . . . . . . . . . . . YOUR NAME
... 7. Suppose you lived on the Moon where there is essentially no atmosphere. Label the following statements as (T)rue or (F)alse: F The Sun would appear redder (compared to as seen from the Earth) during the day. T The color of the sky (looking away from the Sun during the day) would be black. F At su ...
... 7. Suppose you lived on the Moon where there is essentially no atmosphere. Label the following statements as (T)rue or (F)alse: F The Sun would appear redder (compared to as seen from the Earth) during the day. T The color of the sky (looking away from the Sun during the day) would be black. F At su ...
Gravity
... the sun to the Earth. Which of the following best describes the gravitational influence of Vega on Earth? 1. It is roughly equal to that of the sun. 2. Its influence is greater than that of the sun. 3. Its influence is small because of its distance. 4. It influences the magnitude of Earth’s mass. ...
... the sun to the Earth. Which of the following best describes the gravitational influence of Vega on Earth? 1. It is roughly equal to that of the sun. 2. Its influence is greater than that of the sun. 3. Its influence is small because of its distance. 4. It influences the magnitude of Earth’s mass. ...
Assignment 2 - utoledo.edu
... ____ 33. In Ptolemy's system the planets orbit the Earth and not the Sun. How did the system explain the retrograde motion of planets like Jupiter? a. the planets were not moving along the ecliptic but all over the celestial sphere b. the planets moved in very elongated ellipses, and their speed i ...
... ____ 33. In Ptolemy's system the planets orbit the Earth and not the Sun. How did the system explain the retrograde motion of planets like Jupiter? a. the planets were not moving along the ecliptic but all over the celestial sphere b. the planets moved in very elongated ellipses, and their speed i ...
File - SOCIAL SCIENCE
... SPACE TELESCOPES go far out into space and send information and photographs back to Earth. ...
... SPACE TELESCOPES go far out into space and send information and photographs back to Earth. ...
class04
... model, but still based on perfect circles. • Tycho Brahe (1546-1601) “If I had believed that we could made carefulignore observations these eight minutes but [of arc], would could Inot detect have patched up myEarth’s hypothesis motion. accordingly. But, since it was not • Kepler Brahe’s data permis ...
... model, but still based on perfect circles. • Tycho Brahe (1546-1601) “If I had believed that we could made carefulignore observations these eight minutes but [of arc], would could Inot detect have patched up myEarth’s hypothesis motion. accordingly. But, since it was not • Kepler Brahe’s data permis ...
Across 2. a slightly cooler region on the surface of the sun, caused
... 131. what happens to light when a star is moving away from us quickly 132. the cause of the seasons on Earth 136. this star's name is latin for "female warrior" 141. what the sun does to hydrogen to create energy 142. the most dangerous and energetic of light waves 143. constellation we call "the ra ...
... 131. what happens to light when a star is moving away from us quickly 132. the cause of the seasons on Earth 136. this star's name is latin for "female warrior" 141. what the sun does to hydrogen to create energy 142. the most dangerous and energetic of light waves 143. constellation we call "the ra ...
Exploring the Moon and Stars
... show little or no change in their relative position to one another during the span of a human lifetime. • Some constellations and stars appear in the night only at certain times of the year. • Familiar constellations and stars can be used to locate and identify unfamiliar stars and star ...
... show little or no change in their relative position to one another during the span of a human lifetime. • Some constellations and stars appear in the night only at certain times of the year. • Familiar constellations and stars can be used to locate and identify unfamiliar stars and star ...
... waning- when the moon is getting smaller/less light. waxing- when the moon is getting larger/brighter. telescope- a tool that makes objects appear larger. elliptical- an oval/egg shaped orbit. lunar- means moon. Pluto- a former planet that is the smallest and farthest in our solar system. Jupiter- l ...
Lecture #2 - Personal.psu.edu
... Astronomical unit: mean distance from Earth to Sun First measured during transits of Mercury and Venus, using triangulation ...
... Astronomical unit: mean distance from Earth to Sun First measured during transits of Mercury and Venus, using triangulation ...
Solar System Test Review - Garnet Valley School District
... 7. The moon revolves around Earth in _________________________. This causes the moon to rise (and set) approximately _________________________later each day. 8. A _________________________occurs when the moon passes through the earth’s shadow. It may only occur during a _________________________ pha ...
... 7. The moon revolves around Earth in _________________________. This causes the moon to rise (and set) approximately _________________________later each day. 8. A _________________________occurs when the moon passes through the earth’s shadow. It may only occur during a _________________________ pha ...
science - TCDSB.org
... The Earth rotates once every 24 hours. Each time the Earth rotates we have one day and one night. When we are on the sun side of the earth, we have daylight. When we rotate away from the sun, we have night. ...
... The Earth rotates once every 24 hours. Each time the Earth rotates we have one day and one night. When we are on the sun side of the earth, we have daylight. When we rotate away from the sun, we have night. ...
Destination Antarctica Study Buddy
... I can explain why the positions of the Earth, moon, sun and stars change over time. Because the Earth orbits the sun and the moon orbits the Earth, our views of the night sky change in their positions change over time. Stars also change in position over time because the Milky Way galaxy is also rota ...
... I can explain why the positions of the Earth, moon, sun and stars change over time. Because the Earth orbits the sun and the moon orbits the Earth, our views of the night sky change in their positions change over time. Stars also change in position over time because the Milky Way galaxy is also rota ...
Minerals
... In NYS, the sun is almost always in the southern sky; therefore shadows always point north. For anything about seasons: IT’S ALL IN THE TILT – 23 ½ o Earth’s eccentricity is very slight, so it is not quite a circle, it’s an oblate sphere or a slightly eccentric ellipse; BUT . . . A diagram of Earth’ ...
... In NYS, the sun is almost always in the southern sky; therefore shadows always point north. For anything about seasons: IT’S ALL IN THE TILT – 23 ½ o Earth’s eccentricity is very slight, so it is not quite a circle, it’s an oblate sphere or a slightly eccentric ellipse; BUT . . . A diagram of Earth’ ...
exam_1fall_01
... Use Kepler's third law to estimate Vulcan’s (see part b above) orbital period. Show your setup and work. 27. a) The Greeks rejected the heliocentric theory based on the parallax test. Describe their reasoning. (4 pts.) b) How did the work of Tycho, Kepler, and Galileo contribute to supporting the he ...
... Use Kepler's third law to estimate Vulcan’s (see part b above) orbital period. Show your setup and work. 27. a) The Greeks rejected the heliocentric theory based on the parallax test. Describe their reasoning. (4 pts.) b) How did the work of Tycho, Kepler, and Galileo contribute to supporting the he ...
File
... 36. The Great Red Spot is a “storm” in the upper cloud layers of the planet a) Jupiter. b) Saturn c) Uranus d) Neptune 37. The Great Dark Spot is a prominent cloud feature in the upper cloud layers of the planet a) Jupiter. b) Saturn c) Uranus d) Neptune e) The Great Dark Spot is not a recognized cl ...
... 36. The Great Red Spot is a “storm” in the upper cloud layers of the planet a) Jupiter. b) Saturn c) Uranus d) Neptune 37. The Great Dark Spot is a prominent cloud feature in the upper cloud layers of the planet a) Jupiter. b) Saturn c) Uranus d) Neptune e) The Great Dark Spot is not a recognized cl ...
Core Theme 3: The Solar System
... There will be some Penumbral lunar eclipses coming up, but as the Moon will not pass through the main part of the Earth's shadow, there is not much to see, and if you didn't know that an eclipse was taking place you would not be aware of it. So we will have to wait for a decent lunar eclipse until ...
... There will be some Penumbral lunar eclipses coming up, but as the Moon will not pass through the main part of the Earth's shadow, there is not much to see, and if you didn't know that an eclipse was taking place you would not be aware of it. So we will have to wait for a decent lunar eclipse until ...
Full moon
... • Waxing – lit portion of the moon gets bigger each day, lit on the right side. • Waning – lit portion of the moon gets smaller each day, lit on the left side. • Crescent – less than half of the moon’s face is lit (excluding new moon). • Gibbous – more than half of the moon’s face is lit (excluding ...
... • Waxing – lit portion of the moon gets bigger each day, lit on the right side. • Waning – lit portion of the moon gets smaller each day, lit on the left side. • Crescent – less than half of the moon’s face is lit (excluding new moon). • Gibbous – more than half of the moon’s face is lit (excluding ...
Homework 2 (Due Sept 18, 2014)
... b. Find Jupiter’s mass from the fact that its moon Io orbits every 42.5 hours at an average distance of 422,000 km.! c. You discover a planet orbiting a distant star that has about the same mass as the Sun, with an orbital period of 63 days. What is the planet’s orbital distance?! d. Pluto’s moon Ch ...
... b. Find Jupiter’s mass from the fact that its moon Io orbits every 42.5 hours at an average distance of 422,000 km.! c. You discover a planet orbiting a distant star that has about the same mass as the Sun, with an orbital period of 63 days. What is the planet’s orbital distance?! d. Pluto’s moon Ch ...
Planetary Motion
... Solstice: A solstice is an astronomical event that happens twice each year, when the tilt of the Earth's axis is most inclined toward or away from the Sun Equinox: An equinox occurs twice a year, when the tilt of the Earth's axis is inclined neither away from nor towards the Sun, the centre of the S ...
... Solstice: A solstice is an astronomical event that happens twice each year, when the tilt of the Earth's axis is most inclined toward or away from the Sun Equinox: An equinox occurs twice a year, when the tilt of the Earth's axis is inclined neither away from nor towards the Sun, the centre of the S ...
Earth Moon Sun System PPT
... away from Earth than the moon – this is what makes the two objects the same size in the sky. • Solar eclipses occur when the moon passes between the Sun and Earth. • Not everyone gets to see a solar eclipse b/c the moon’s shadow that falls on Earth is very small (only 167 miles wide) and moves quick ...
... away from Earth than the moon – this is what makes the two objects the same size in the sky. • Solar eclipses occur when the moon passes between the Sun and Earth. • Not everyone gets to see a solar eclipse b/c the moon’s shadow that falls on Earth is very small (only 167 miles wide) and moves quick ...
Earth Moon Sun System PPT
... away from Earth than the moon – this is what makes the two objects the same size in the sky. • Solar eclipses occur when the moon passes between the Sun and Earth. • Not everyone gets to see a solar eclipse b/c the moon’s shadow that falls on Earth is very small (only 167 miles wide) and moves quick ...
... away from Earth than the moon – this is what makes the two objects the same size in the sky. • Solar eclipses occur when the moon passes between the Sun and Earth. • Not everyone gets to see a solar eclipse b/c the moon’s shadow that falls on Earth is very small (only 167 miles wide) and moves quick ...
CHAPTER 13: GRAVITATIONAL INTERACTIONS 13.1
... g is the gravitational field vector They are all different quantities that are related G and g have the same magnitude and their units are equivalent: N/kg = m/s2 g = GM/R2 g = 9.8 N/kg is valid only near the planet’s surface as R increases, g decreases The strength of Earth’s gravitational field is ...
... g is the gravitational field vector They are all different quantities that are related G and g have the same magnitude and their units are equivalent: N/kg = m/s2 g = GM/R2 g = 9.8 N/kg is valid only near the planet’s surface as R increases, g decreases The strength of Earth’s gravitational field is ...
Document
... • In the 3rd Century B.C., a Greek, Aristarchus of Samos, figured out a way to measure the relative sizes and distances of the Moon and Sun. • He noticed that when the Moon was eclipsed by the Earth (월식) we can see the Earth's shadow creep across the face of the Moon. Earth's shadow is circular, and ...
... • In the 3rd Century B.C., a Greek, Aristarchus of Samos, figured out a way to measure the relative sizes and distances of the Moon and Sun. • He noticed that when the Moon was eclipsed by the Earth (월식) we can see the Earth's shadow creep across the face of the Moon. Earth's shadow is circular, and ...